Description of accretion induced outflows from ultra-luminous sources to under luminous AGNs

Abstract

We study the energetics of the accretion-induced outflow and then plausible jet around black holes/compact objects using a newly developed disc-outflow coupled model. Inter-connecting dynamics of outflow and accretion essentially upholds the conservation laws. The energetics depend strongly on the viscosity parameter a and the cooling factor f which exhibit several interesting features. The bolometric luminosities of ultra-luminous X-ray binaries (e.g. SS433) and family of highly luminous AGNs and quasars can be reproduced by the model under the super-Eddington accretion flows. Under appropriate conditions, lowluminous AGNs (e.g. Sagittarius A ) also fit reasonably well with the luminosity corresponding to a sub- Eddington accretion flow with f ! 1.